dc.contributor.author |
Mavraganis, AG |
en |
dc.date.accessioned |
2014-03-01T01:07:28Z |
|
dc.date.available |
2014-03-01T01:07:28Z |
|
dc.date.issued |
1989 |
en |
dc.identifier.issn |
0004-640X |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/10006 |
|
dc.subject |
Degeneration |
en |
dc.subject.classification |
Astronomy & Astrophysics |
en |
dc.title |
Extreme models of magnetic-binary systems |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1007/BF00640496 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1007/BF00640496 |
en |
heal.language |
English |
en |
heal.publicationDate |
1989 |
en |
heal.abstract |
In this article the author investigates the models of a magnetic-binary system produced by varying the two basic parameters of it, namely the one determining the electromagnetic character of the system and the mass parameter. At the limit of these parameters he states again the Störmer's problem in a general form, by introducing some new affected terms due to the degeneration of the magnetic-binary problem. © 1989 Kluwer Academic Publishers. |
en |
heal.publisher |
Kluwer Academic Publishers |
en |
heal.journalName |
Astrophysics and Space Science |
en |
dc.identifier.doi |
10.1007/BF00640496 |
en |
dc.identifier.isi |
ISI:A1989AT09800015 |
en |
dc.identifier.volume |
159 |
en |
dc.identifier.issue |
1 |
en |
dc.identifier.spage |
153 |
en |
dc.identifier.epage |
156 |
en |